中文

高分辨率X射线成像科学

高能天体物理现象 2026-06-26 v1
作者: H. L. Marshall , K. Weaver , M. Schattenburg , B. Binder , H. M. Günther , S. J. Wolk , K. G. Stassun , S. J. Gunderson , R. Pandey , L. Valencic , P. Draghis , J. Hare , M. Balakrishnan , T. Boztepe , P. Gandhi , T. Holland-Ashford , T. Maccarone , M. Reynolds , M. Sobolewska , R. Tanner , J. Cann , P. Chakraborty , B. Coleman , S. DiKerby , R. Gamble , J. Irwin , P. Maksym , J. McKaig , E. Perlman , D. Pooley , S. Randall , H. Russell , A. Sarkar , S. Turriziani , K. -W. Wong , K. Whalen , D. Haggard
在 arXiv 上查看 ↗ PDF ↗

摘要

本报告总结了Hi-ReX科学分析小组关于超高角分辨率X射线天文台的潜在研究。报告提出了许多潜在的科学案例，涵盖从太阳系行星和系外行星到超大质量黑洞和宇宙学等一系列天体物理课题。这些案例证明了X射线成像超越当前能力、面向毫角秒和微角秒角尺度的价值。目前，最好的X射线成像望远镜——钱德拉X射线天文台的能力与电磁波谱中其他仪器相比存在成像差距。下一代超高角分辨率X射线成像将弥合这一差距，并改变我们对宇宙和基础物理的理解。

关键词

X射线成像 高角分辨率 天文台 天体物理学 钱德拉 宇宙学 系外行星

引用

@article{arxiv.2606.28138,
  title  = {Science of High Resolution X-ray Imaging},
  author = {H. L. Marshall and K. Weaver and M. Schattenburg and B. Binder and H. M. Günther and S. J. Wolk and K. G. Stassun and S. J. Gunderson and R. Pandey and L. Valencic and P. Draghis and J. Hare and M. Balakrishnan and T. Boztepe and P. Gandhi and T. Holland-Ashford and T. Maccarone and M. Reynolds and M. Sobolewska and R. Tanner and J. Cann and P. Chakraborty and B. Coleman and S. DiKerby and R. Gamble and J. Irwin and P. Maksym and J. McKaig and E. Perlman and D. Pooley and S. Randall and H. Russell and A. Sarkar and S. Turriziani and K. -W. Wong and K. Whalen and D. Haggard},
  journal= {arXiv preprint arXiv:2606.28138},
  year   = {2026}
}

备注

This is a report generated in response to a call by the X-ray Science Interest Group of the NASA Physics of the Cosmos Program Analysis Group (PhysPAG). The report summarizes the reports of 5 working groups, which will provide more details of each science case and be published independently. Links will be provided when available